This paper is devoted to solve the galactic rotation problem based on Modified Newtonian Dynamics (MOND). It addresses a new fundamental constant a0, called the acceleration constant, at which acceleration scale of Newton's second law fails to hold. It is an indication of a breakdown of classical Newtonian dynamics. In this respect, we choose the HI observations of a late type galaxy, ESO138-G014, to test the rotation curve within the MOND framework which leads to "MOND RC". We ask whether ESO138-G014 is compatible with MOND or dark matter is still favorable for the galactic rotation problem. © 2013 AIP Publishing LLC.

The study of rotation curve with MOND for ESO138-G014 / Hashim, N.; Salucci, P.; Abidin, Z. Z.. - 1528:(2013), pp. 70-75. (Intervento presentato al convegno 2012 National Physics Conference, PERFIK 2012 tenutosi a Bukit Tinggi, Pahang, mys nel 2012) [10.1063/1.4803571].

The study of rotation curve with MOND for ESO138-G014

Salucci P.;
2013-01-01

Abstract

This paper is devoted to solve the galactic rotation problem based on Modified Newtonian Dynamics (MOND). It addresses a new fundamental constant a0, called the acceleration constant, at which acceleration scale of Newton's second law fails to hold. It is an indication of a breakdown of classical Newtonian dynamics. In this respect, we choose the HI observations of a late type galaxy, ESO138-G014, to test the rotation curve within the MOND framework which leads to "MOND RC". We ask whether ESO138-G014 is compatible with MOND or dark matter is still favorable for the galactic rotation problem. © 2013 AIP Publishing LLC.
2013
AIP Conference Proceedings
1528
70
75
Hashim, N.; Salucci, P.; Abidin, Z. Z.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11767/117130
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